Observations of the deeply eclipsing dwarf nova GY Cnc

被引：0
|
作者：
Katysheva, NA [1 ]
Shugarov, SY [1 ]
机构：
[1] Sternberg State Astron Inst, Moscow, Russia
来源：
ASTROPHYSICS AND SPACE SCIENCE | 2005年 / 296卷 / 1-4期
关键词：
binary stars; cataclysmic variables; X-ray source;
D O I：
10.1007/s10509-005-4892-2
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We present photometric measurements of the eclipsing dwarf nova and X-ray source GY Cnc. The observations were collected during outbursts and in quiescence. The investigation of plates from the Sonneberg archive showed that the mean outburst interval is about 210-270 days, that the outburst is very fast, and lasts for about 5 days.
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页码：469 / 472
页数：4
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